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Fig. 3

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Spectra obtained with the radiative transfer code (model, in red) overlaid to the observations (black) for N2 H+ (1–0) and (3–2) lines. The columns refer to the three models: in the left panels, in the central panels, and in the right ones. The corrective factors fcorr used to modify the whole abundance profile to match the observed fluxes is indicated above the top panel of each column. All models are at t = 106 yr.

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